The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …

The formation of a protostellar disc is a natural outcome during the star formation process.
As gas in a molecular cloud core collapses under self-gravity, the angular momentum of the …

Characterizing the physical properties of dust grains in a protoplanetary disk is critical to
comprehending the planet formation process. Our study presents Atacama Large Millimeter …

We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet
systems, obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) at 870 μm …

The mechanism for producing polarized emission from protostellar disks at (sub) millimeter
wavelengths is currently uncertain. Classically, polarization is expected from non-spherical …

Dust particle sizes constrained from dust continuum and polarization observations by radio
interferometry are inconsistent by at least an order of magnitude. Motivated by porous dust …

Abstract We present 0 farcs 25 resolution (35 au) ALMA 1.3 mm dust polarization
observations for 37 young stellar objects (YSOs) in the Ophiuchus molecular cloud. These …

We present ALMA images of the sub-mm continuum polarization and spectral index of the
protoplanetary ringed disc HD163296. The polarization fraction at 870 µm is measured to …

We present the full disk-fit results VANDAM survey of all Class 0 and I protostars in the
Perseus molecular cloud. We have 18 new protostellar disk candidates around Class 0 and I …

We present 870 μm ALMA observations of polarized dust emission toward the Class II
protoplanetary disk IM Lup. We find that the orientation of the polarized emission is along the …